Reference : CPD - 59 deg 2857 - A new red variable star
Scientific journals : Article
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/28037
CPD - 59 deg 2857 - A new red variable star
English
Gosset, Eric mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Groupe d'astrophysique des hautes énergies (GAPHE) >]
Hutsemekers, Damien mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS) >]
Surdej, Jean mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS) >]
1985
Publications of the Astronomical Society of the Pacific [=PASP]
University of Chicago Press
97
67-71
Yes (verified by ORBi)
International
0004-6280
1538-3873
Chicago
USA
[en] LATE STARS ; LIGHT CURVE ; PECULIAR STARS ; RED GIANT STARS ; STELLAR SPECTRA ; VARIABLE STARS ; EMISSION SPECTRA ; SEMIREGULAR VARIABLE STARS ; STELLAR SPECTROPHOTOMETRY ; UBV SPECTRA
[en] Two (C3 and C4) of the four comparison stars monitored during the photometric study of the peculiar emission-line star GG Car (Gosset et al., 1984) have been found to be variable. Available photometric and spectroscopic data allow us to identify C4 with CPD - 59 deg 2857 and classify it as a late-type giant (M3-4 III) belonging to the red variable stars of the semiregular or irregular type.
Researchers ; Professionals
http://hdl.handle.net/2268/28037
10.1086/131498
http://adsabs.harvard.edu/abs/1985PASP...97...67G
The authors thank SAO/NASA ADS Astronomy Abstract Service for their deposit authorization.

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